You Spin Me Right Round: A Magnetic Avalanche in the Solar Corona
Can a chain reaction in the magnetic field supply the energy to keep the solar atmosphere at a temperature of several million Kelvin?
Studying the Population of Variable Objects in the Dark Energy Survey
Today’s undergraduate research post is seeking to automatically identify variable stars in the upcoming all sky survey, LSST. Read on to find out more!
The Beating Heart(-Shaped Region) of Pluto
Like human, like dwarf planet – it turns out Pluto’s heart has a “heartbeat.”
Spin-teresting Effects of Binary Star Formation
We see that many stars have a buddy star or two i.e. they are a binary or multi-star system. This paper addresses the question: How in the heck does that happen?
Modeling Supernovae Feedback as a Galactic Fountain
Stellar feedback can drive a galactic fountain by pushing out gas that later falls back in.
When Do Stars Form? Simulating Dynamic Star Formation Efficiencies in Giant Molecular Clouds
Observations of Giant Molecular Clouds (GMCs) yield large scatters in star formation efficiencies. Simulations in this work show that much of this scatter may stem from the fact we observe GMCs at different evolutionary stages driven by stellar feedback.